Fig. 7
Left: AGC 198606, AGC 249525 and AGC 249565 (the three galaxy candidates) shown on the Baryonic Tully-Fisher relation (BTFR) of McGaugh (2012) with Leo P and the SHIELD galaxies (Bernstein-Cooper et al. 2014; McNichols et al. 2016) shown for extension to low rotational velocities. Right: UCHVCs of A13 (open circles) and this work (open symbols, same colors and shapes as in Figs. 2 and 3) shown on the BTFR based on their single-dish ALFALFA properties. The galaxy candidates are shown based on their rotation velocities derived in this work.
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